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Dust in FIR-bright ADF-S galaxies

Published online by Cambridge University Press:  09 February 2015

K. Małek
Affiliation:
Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, 464-8602 Nagoya, Japan email: malek@cft.edu.pl National Centre for Nuclear Research, ul. Hoża 69, 00-681 Warszawa, Poland
A. Pollo
Affiliation:
National Centre for Nuclear Research, ul. Hoża 69, 00-681 Warszawa, Poland The Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30-244 Kraków, Poland
T. T. Takeuchi
Affiliation:
Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, 464-8602 Nagoya, Japan email: malek@cft.edu.pl
V. Buat
Affiliation:
Laboratoire d'Astrophysique de Marseille, OAMP, Universite Aix-Marseille, CNRS, 38 rue Frerdeic Joliot-Curie, 13388 Marseille, cedex 13, France
D. Burgarella
Affiliation:
Laboratoire d'Astrophysique de Marseille, OAMP, Universite Aix-Marseille, CNRS, 38 rue Frerdeic Joliot-Curie, 13388 Marseille, cedex 13, France
M. Malkan
Affiliation:
Department of Physics and Astronomy, University of California, Los Angeles, CA 90024, USA
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Abstract

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Multiwavelength Spectral Energy Distributions (SEDs) of far-infrared (FIR) galaxies detected in the AKARI South Ecliptic Poles Survey (ADF-S) allow to trace differences between [Ultra]-Luminous Infrared Galaxies ([U]LIRGS) and other types of star-forming galaxies (SF).

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Małek, K., Pollo, A., Takeuchi, T. T., et al. 2013, EPS, Special Issue Cosmic Dust V, 65, 1101Google Scholar
Małek, K., Pollo, A., Takeuchi, T. T., et al. 2014, A&A 562 id.A15Google Scholar
Noll, S., Burgarella, D., Giovannoli, E., et al. 2009, A&A, 507, 1793Google Scholar